Relation between the ratio of rest-frame 2 μm point source (PS) luminosity to total (PSF + Sérsic) 2 μm luminosity (a) and PS luminosity (b) as a function of the 0.5−7.0 keV X-ray luminosity. In each panel we show the Spearman rank correlation coefficient (r_s) for the relations, a running median (grey squares) in bins of 1 dex in X-ray luminosity. We exclude sources in panel b with a PS to total luminosity ratio of less than 20%. We further show the one-to-one relation (dashed black line) and overlay nearby (z ∼ 0.01) AGNs from Burtscher et al. (2015), as well as the 6 μm – X-ray luminosity relations from Mateos et al. (2015) for z ≃ 0.2−2.8 AGN and higher-redshift quasars from Chen et al. (2017), as well as the MIRI-SMILES X-ray sources from Lyu et al. (2024). Whilst we identify a strong (r = 0.73) correlation between NIR point-source luminosity and X-ray luminosity in our samples, at log₁₀(L_Xc) ≤ 43 erg s⁻¹, we identify higher 2 μm PS luminosities than other studies, with no strong correlation with column density (N_H).